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<h2 class="sec">Online Material</h2>

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<h2 class="sec"><a name="SECTION000110000000000000000"></a><A NAME="a:cospectra"></A>
Appendix A: New CO spectra
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<tr><td><!-- init Label --><A NAME="rand_co1">&#160;</A><!-- end Label--><A NAME="2910"></A><A NAME="figure1889"
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<td class="img-txt"><span class="bold">Figure A.1:</span><p>
New observations of circumstellar CO line emission. The source name is shown to the <I> upper left</I>, and the transition observed and the telescope used is shown to the <I> upper right</I> of each frame. LSR velocity scales are used.</p></td>
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<td class="img-txt"><span class="bold">Figure A.1:</span><p>
continued.</p></td>
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<td class="img-txt"><span class="bold">Figure A.1:</span><p>
continued.</p></td>
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<A NAME="COintensities1"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/20/aa11730-09/tableA.1.html"><span class="bold">Table A.1:</span></a>&#160;&#160;
Observational results of circumstellar CO radio lineemission.</p>
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<h2 class="sec"><a name="SECTION000120000000000000000"></a><A NAME="a:siospectra"></A>
Appendix B: New SiO spectra
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<A NAME="SiOintensities1"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/20/aa11730-09/tableB.1.html"><span class="bold">Table B.1:</span></a>&#160;&#160;
Observational results of circumstellar SiO radio lineemission.</p> 

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<A NAME="SiOintensitiesm1"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/20/aa11730-09/tableB.2.html"><span class="bold">Table B.2:</span></a>&#160;&#160;
Observational results of circumstellar SiO(<I>J</I>&nbsp;=&nbsp;2-1, <I>v</I>=1) emission.</p>
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<td class="img-txt"><span class="bold">Figure B.1:</span><p>
New observations of circumstellar SiO line emission (<I>v</I>=0). The source name is shown to the <I> upper left</I>, and the transition observed and the telescope used is shown to the <I> upper right</I> of each frame. LSR velocity scales are used.</p></td>
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continued.</p></td>
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<td class="img-txt"><span class="bold">Figure B.2:</span><p>
New observations of circumstellar SiO line emission (<I>v</I>=1). The source name is shown to the <I> upper left</I>, and the transition observed and the telescope used is shown to the <I> upper right</I> of each frame. LSR velocity scales are used.</p></td>
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